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July 24, 2009 : Workshop on the Mid-infrared Instrument for TAO 6.5m telescope

A workshop on the mid-infrared instrument for TAO 6.5m telescope (TAOMIR) was held on July 24, 2009. Sufficient exchanges of opinions about the specifications, the performances, and the scientific cases of the TAOMIR were conducted. We continue to develop the TAOMIR in order to be a widely used instrument for many astronomers.

TAO中間赤外線装置ワークショップの様子 TAO中間赤外線装置ワークショップの様子
▲ TAOMIR workshop
Date:2009/07/24(Fri) 11:00 - 18:00
Venue:Lecture room at the Institute of Astronomy, UT
Program:11:00-11:05RemarksMiyata
Details of the instruments
11:05-11:20MAX38: a prototype camera of the TAOMIRNakamura, Asano
11:20-11:50TAOMIRMiyata
11:50-12:45Lunch
Stars
12:45-13:00Imaging/Spectroscopic Monitoring of nearby variable stars in MIRIta
13:00-13:15Mira variables in the galactic center seen by TAOMatsunaga
13:15-13:30Investigations of MOLsphereTanabe
Star and Planet formation
13:30-13:45Observations of dust around young starsFujiwara
13:45-14:00Monitoring observations of disks, and some comments on the instrument spec.Kataza
14:00-14:15Massive star formationOkamoto
14:15-14:30Break
Interstellar Medium
14:30-14:45Science cases of MIR polarimetryHonda
14:45-15:00Interstellar medium studied with TAOMIRSakon
Solar system
15:00-15:15Small bodies in the solar system studied with TAOMIROtsubo
15:15-15:30MIR imaging observations of cometsIshiguro
15:30-15:45Planetary magnetosphere observed in MIRYoneda
Synergy with Radio obsevations
15:45-16:00Synergy of TAOMIR and ALMA/ASTEKohno
16:00-16:15Break
Extragalaxy
16:15-16:30Mass estimation of CDM subhalo with MIR monitoring observationsMinezakiMinezaki
16:30-16:45Follow-ups of MIR all sky survey: Searching for dust obscured AGNsOyabu
16:45-17:00Break
TAOMIR Science WG
17:00-17:15Summary and TAOMIR science WGSako
Discussion
17:15-18:00DiscussionMiyata